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s
s
TT
==
0
therefore,
(42c)
rs
,
rs
,
B
B
Decomposition Eq. (42a) is valuable in the study of electromagnetic an-
gular momentum; here, it came out as a consequence of the spintensor
concept Eq. (40b).
It can be proven that
(
)
2
(
)
q
4
b
sar
KwD
=
=
41.c
,
(43a)
4
sar
B
,
b
where
D
is a tensor employed by Synge [7] in another context:
ijrm
Dg k k
=
g
k k
g
k k
g
k k
(43b)
sarb
rs
a
b
ab
r
s
ar
s
b
sb
a
r
Identity Eq. (43a) was obtained by Rowe [53].
Weert did not study Eq. (35a); this analysis was considered in [54-61]
to determine a nonlocal superpotential (it depends on integrals over the
world line) for the radiative part:
a
TK
=
(44a)
rs
sr a
,
R
R
with
)
(
()
τ
τ
() ()
() ()()
σθ
σθβ
K
X
i
=
qF
[
p
p
a
a
v d
γ
+
p
a
a
e
d
γ
() ()
()
sc
r
r
σθ
β
scr
0
0
R
(44b)
τ
τ
()
σ
2
2
avd
γ
p
ae d
γ
],
σ θ β
,
,
=
1, 2, 3
()
r
r
σ
0
0
τ
is the proper time in the retarded point
associated to X . Trying out Eq. (44a) brings into relevance the identities
Eq. (24); the integrals in Eq. (44b) indicate the nonlocal character of radia-
tive superpotential; besides, if the four-acceleration
where
( er
is the Fermi triad and
σ
a is annulated, then
= which was to be expected due to Eq. (26). When obtaining Eq. (44),
transport Eq. (9a) is basic; never before had the great value of the Fermi
triad been shown in electrodynamics.
K
0
ijc
R
 
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